A dataset provided by the European Space Agency

Name: Study of the chemical enrichment in a massive hot cooling-flow cluster
Published: 2009-09-30T00:00:00Z

Proposal ID	055178
Title	Study of the chemical enrichment in a massive hot cooling-flow cluster
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551780201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551780301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551780401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551780501
DOI	https://doi.org/10.5270/esa-rltoh55
Principal Investigator, PI	Mr Norbert Werner
Abstract	Clusters of galaxies are excellent laboratories for the study of thenucleosynthesis and chemical enrichment history of the Universe. These studiesare currently biased toward relatively cooler (2-4 keV) clusters. However, theenrichment history of the massive hot clusters might be different from that ofthe smaller and cooler systems. Therefore, we propose to enlarge the sample ofclusters observed with the RGS on XMM-Newton with Abell 2029, a hot luminousmassive cluster with a cooling core. Despite of the high mass of this system,the cool gas in the core will allow us to measure the abundances of manyelements. A deep (130 ks) observation will provide us with EPIC and RGS spectraof excellent statistics, which allows us to accurately measure the abundances O, Ne, Mg, Si, S, Ar, Ca, Fe, and Ni.
Publications	Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations \|Planck Collaboration, Ade, P. A. R., et al. \| A&A \| 536-11 \| 2011 \| 2011A&A...536A..11P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...536A..11P Star Formation Efficiency in the Cool Cores of Galaxy Clusters \|McDonald, Michael, Veilleux, Sylvain, et al. \| ApJ \| 734-95 \| 2011 \| 2011ApJ...734...95M \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...734...95M Cold fronts in galaxy clusters \|Ghizzardi, S., Rossetti, M., \| A&A \| 516-32 \| 2010 \| 2010A&A...516A..32G \| http://ui.adsabs.harvard.edu/#abs/2010A&A...516A..32G Inhomogeneous metal distribution in the intracluster medium \|Lovisari, L., Schindler, S., \| A&A \| 528-60 \| 2011 \| 2011A&A...528A..60L \| http://ui.adsabs.harvard.edu/#abs/2011A&A...528A..60L Constraints on turbulent velocity broadening for a sample of clusters, groups and elliptical galaxies using XMM-Newton \|Sanders, J. S., Fabian, A. C., \| MNRAS \| 410-1797 \| 2011 \| 2011MNRAS.410.1797S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.410.1797S Revealing O VII from stacked X-ray grating spectra of clusters, groups and elliptical galaxies \|Sanders, J. S., Fabian, A. C., \| MNRAS \| 412-35 \| 2011 \| 2011MNRAS.412L..35S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.412L..35S An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F On the Origin of the Extended Halpha Filaments in Cooling Flow Clusters \|McDonald, Michael, Veilleux, Sylvain, et al. \| ApJ \| 721-1262 \| 2010 \| 2010ApJ...721.1262M \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...721.1262M Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L The cool-core bias in X-ray galaxy cluster samples. I. Method and application to HIFLUGCS \|Eckert, D., Molendi, S., \| A&A \| 526-79 \| 2011 \| 2011A&A...526A..79E \| http://ui.adsabs.harvard.edu/#abs/2011A&A...526A..79E A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi, J. A., Albacete Colombo, J. F., et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C Characterization of Intracluster Medium Temperature Distributions of 62 Galaxy Clusters with XMM-Newton \|Frank, K. A., Peterson, J. R., et al. \| ApJ \| 764-46 \| 2013 \| 2013ApJ...764...46F \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...764...46F Velocity width measurements of the coolest X-ray emitting material in the cores of clusters, groups and elliptical galaxies \|Sanders, J. S., Fabian, A. C., \| MNRAS \| 429-2727 \| 2013 \| 2013MNRAS.429.2727S \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.429.2727S Planck intermediate results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect \|Planck Collaboration, Ade, P. A. R., et al. \| A&A \| 550-131 \| 2013 \| 2013A&A...550A.131P \| http://ui.adsabs.harvard.edu/#abs/2013A&A...550A.131P Insight into Active Galactic Nucleus and Host Galaxy Co-evolution from Hard X-Ray Emission \|Wang, J., Zhou, X. L., \| ApJ \| 768-176 \| 2013 \| 2013ApJ...768..176W \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...768..176W Galaxy Cluster Baryon Fractions Revisited \|Gonzalez, Anthony H., Sivanandam, Suresh, et al. \| ApJ \| 778-14 \| 2013 \| 2013ApJ...778...14G \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...778...14G The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S Confirming the thermal Comptonization model for black hole X-ray emission in the low-hard state \|Castro, M., D.Amico, F., et al. \| A&A \| 569-82 \| 2014 \| 2014A&A...569A..82C \| http://ui.adsabs.harvard.edu/#abs/2014A&A...569A..82C Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y XMM-Newton and Chandra cross-calibration using HIFLUGCS galaxy clusters . Systematic temperature differences and cosmological impact \|Schellenberger, G., Reiprich, T. H., et al. \| A&A \| 575-30 \| 2015 \| 2015A&A...575A..30S \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..30S Chemical Enrichment RGS cluster Sample (CHEERS): Constraints on turbulence \|Pinto, Ciro, Sanders, Jeremy S., et al. \| A&A \| 575-38 \| 2015 \| 2015A&A...575A..38P \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..38P Origin of central abundances in the hot intra-cluster medium. I. Individual and average abundance ratios from XMM-Newton EPIC \|Mernier, F., de Plaa, J., et al. \| A&A \| 592-157 \| 2016 \| 2016A&A...592A.157M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...592A.157M Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti, F., Middei, R., et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Origin of central abundances in the hot intra-cluster medium. II. Chemical enrichment and supernova yield models \|Mernier, F., de Plaa, J., et al. \| A&A \| 595-126 \| 2016 \| 2016A&A...595A.126M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...595A.126M X-Ray Morphological Analysis of the Planck ESZ Clusters \|Lovisari, Lorenzo, Forman, William R., et al. \| ApJ \| 846-51 \| 2017 \| 2017ApJ...846...51L \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...846...51L HICOSMO: cosmology with a complete sample of galaxy clusters - II. Cosmological results \|Schellenberger, G., Reiprich, T. H., \| MNRAS \| 471-1370 \| 2017 \| 2017MNRAS.471.1370S \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.1370S CHEERS: The chemical evolution RGS sample \|de Plaa, J., Kaastra, J. S., et al. \| A&A \| 607-98 \| 2017 \| 2017A&A...607A..98D \| http://ui.adsabs.harvard.edu/#abs/2017A&A...607A..98D Solar abundance ratios of the iron-peak elements in the Perseus cluster \|Hitomi Collaboration, Aharonian, Felix, et al. \| Natur \| 551-478 \| 2017 \| 2017Natur.551..478H \| http://ui.adsabs.harvard.edu/#abs/2017Natur.551..478H Charge exchange in galaxy clusters \|Gu, Liyi, Mao, Junjie, et al. \| A&A \| 611-26 \| 2018 \| 2018A&A...611A..26G \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..26G Mass-invariance of the iron enrichment in the hot haloes of massive ellipticals, groups, and clusters of galaxies \|Mernier, F., de Plaa, J., et al. \| MNRAS \| 478-116 \| 2018 \| 2018MNRAS.478L.116M \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478L.116M Solar chemical composition in the hot gas of cool-core ellipticals, groups, and clusters of galaxies \|Mernier, F., Werner, N., et al. \| MNRAS \| 480-95 \| 2018 \| 2018MNRAS.480L..95M \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480L..95M The non-uniformity of galaxy cluster metallicity profiles \|Lovisari, L., Reiprich, T. H., \| MNRAS \| 483-540 \| 2019 \| 2019MNRAS.483..540L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483..540L Enrichment of the Hot Intracluster Medium: Observations \|Mernier, F., Biffi, V., et al. \| SSRv \| 214-129 \| 2018 \| 2018SSRv..214..129M \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214..129M Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters \|Kozmanyan, Arpine, Bourdin, Herve, et al. \| A&A \| 621-34 \| 2019 \| 2019A&A...621A..34K \| http://ui.adsabs.harvard.edu/#abs/2019A&A...621A..34K Universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample \|Ghirardini, V., Eckert, D., et al. \| A&A \| 621-41 \| 2019 \| 2019A&A...621A..41G \| http://ui.adsabs.harvard.edu/#abs/2019A&A...621A..41G Discovery of Dying Active Galactic Nucleus in Arp 187: Experience of Drastic Luminosity Decline within 104 yr \|Ichikawa, Kohei, Ueda, Junko, et al. \| ApJ \| 870-65 \| 2019 \| 2019ApJ...870...65I \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...870...65I The Galaxy Cluster Mass Scale and Its Impact on Cosmological Constraints from the Cluster Population \|Pratt, G. W., Arnaud, M., et al. \| SSRv \| 215-25 \| 2019 \| 2019SSRv..215...25P \| http://ui.adsabs.harvard.edu/#abs/2019SSRv..215...25P Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters \|Lagana, T. F., Durret, F., \| MNRAS \| 484-2807 \| 2019 \| 2019MNRAS.484.2807L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.484.2807L Searching for cool and cooling X-ray emitting gas in 45 galaxy clusters and groups \|Liu, Haonan, Pinto, Ciro, et al. \| MNRAS \| 485-1757 \| 2019 \| 2019MNRAS.485.1757L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.485.1757L The Fornax3D project: Tracing the assembly history of the cluster from the kinematic and line-strength maps \|Iodice, E., Sarzi, M., et al. \| A&A \| 627-136 \| 2019 \| 2019A&A...627A.136I \| http://ui.adsabs.harvard.edu/#abs/2019A&A...627A.136I Why are some galaxy clusters underluminous?. The very low concentration of the CL2015 mass profile \|Andreon, S., Moretti, A., et al. \| A&A \| 630-78 \| 2019 \| 2019A&A...630A..78A \| http://ui.adsabs.harvard.edu/#abs/2019A&A...630A..78A X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton \|Lovisari, Lorenzo, Schellenberger, Gerrit, et al. \| ApJ \| 892-102 \| 2020 \| 2020ApJ...892..102L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...892..102L X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C Hot Atmospheres of Galaxies, Groups, and Clusters of Galaxies \|Werner, Norbert, Mernier, Fran\\u00e7ois, \| rfma \| 0-279 \| 2020 \| 2020rfma.book..279K \| http://ui.adsabs.harvard.edu/#abs/2020rfma.book..279K Comparing different mass estimators for a large subsample of the Planck-ESZ clusters \|Lovisari, L., Ettori, S., et al. \| A&A \| 644-78 \| 2020 \| 2020A&A...644A..78L \| http://ui.adsabs.harvard.edu/#abs/2020A&A...644A..78L The Metal Content of the Hot Atmospheres of Galaxy Groups \|Gastaldello, Fabio, Simionescu, Aurora, et al. \| Univ \| 7-208 \| 2021 \| 2021Univ....7..208G \| http://ui.adsabs.harvard.edu/#abs/2021Univ....7..208G The thermalization of massive galaxy clusters \|Sereno, Mauro, Lovisari, Lorenzo, et al. \| MNRAS \| 507-5214 \| 2021 \| 2021MNRAS.507.5214S \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.5214S Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z PACT. II. Pressure profiles of galaxy clusters using Planck and ACT \|Pointecouteau, E., Santiago-Bautista, I., et al. \| A&A \| 651-73 \| 2021 \| 2021A&A...651A..73P \| http://ui.adsabs.harvard.edu/#abs/2021A&A...651A..73P A detailed study of the bridge of excess X-ray emission between the galaxy clusters Abell 2029 and Abell 2033 \|Mirakhor, M. S., Walker, S. A., \| MNRAS \| 509-1109 \| 2022 \| 2022MNRAS.509.1109M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.1109M High-resolution X-ray spectroscopy of astrophysical plasmas with X-ray microcalorimeters \|Ezoe, Yuichiro, Ohashi, Takaya, \| RvMPP \| 5-4 \| 2021 \| 2021RvMPP...5....4E \| http://ui.adsabs.harvard.edu/#abs/2021RvMPP...5....4E Studying the merging cluster Abell 3266 with eROSITA \|Sanders, J. S., Biffi, V., et al. \| A&A \| 661-36 \| 2022 \| 2022A&A...661A..36S \| http://ui.adsabs.harvard.edu/#abs/2022A&A...661A..36S A systematic comparison of galaxy cluster temperatures measured with NuSTAR and Chandra \|Wallbank, A. N., Maughan, B. J., et al. \| MNRAS \| 517-5594 \| 2022 \| 2022MNRAS.517.5594W \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517.5594W Heating of the intracluster medium by buoyant bubbles and sound waves \|Iqbal, Asif, Majumdar, Subhabrata, et al. \| MNRAS \| 518-2735 \| 2023 \| 2023MNRAS.518.2735I \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.518.2735I Galaxy clusters in X-rays: the buildup of massive structures in the last 10 Gyrs, and CHEX-MATE \|Ettori, S., Bourdin, H., et al. \| MmSAI \| 93-98 \| 2022 \| 2022MmSAI..93b..98E \| http://ui.adsabs.harvard.edu/#abs/2022MmSAI..93b..98E Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters \|Wicker, R., Douspis, M., et al. \| A&A \| 674-48 \| 2023 \| 2023A&A...674A..48W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A..48W Studying X-ray instruments with galaxy clusters \|Nevalainen, J., Molendi, S., \| A&A \| 676-142 \| 2023 \| 2023A&A...676A.142N \| http://ui.adsabs.harvard.edu/#abs/2023A&A...676A.142N Characterizing the bulk and turbulent gas motions in galaxy clusters \|Dupourqu\\u00e9, Simon, Pointecouteau, Etienne, et al. \| EPJWC \| 257-00015 \| 2022 \| 2022EPJWC.25700015D \| http://ui.adsabs.harvard.edu/#abs/2022EPJWC.25700015D From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2008-07-17T08:01:53Z/2008-08-18T11:50:05Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2009-09-30T00:00:00Z
Keywords	"cool gas", "kev clusters", "abell 2029", "XMM", "xmm newton", "cooler systems", "relatively cooler", "chemical enrichment", "Abell 2029", "massive hot cluster", "cooling core", "deep 130", "XMM-Newton", "EPIC", "rgs spectra", "enrichment history", "chemical enrichment history"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Norbert Werner, 2009, 'Study of the chemical enrichment in a massive hot cooling-flow cluster', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rltoh55